Coagulation of interstellar dust in a turbulent gas

Details Coagulation of interstellar dust in a turbulent gas Coagulation of interstellar dust in a turbulent gas

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57..566k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 57, May-June 1980, p. 566-576.) Soviet Astronomy, vol. 24, May-June 1980, p. 328-334. Translati

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, Gravitational Collapse, Interstellar Matter, Protoplanets, Cosmology, Planetary Evolution, Planetary Nebulae, Solar System, Turbulence Effects

Scientific paper

The physical processes causing the coagulation of dust grains in the contracting protoplanetary clouds in regions of intense turbulent gas movements are discussed. The effects of turbulence are indicated by the presence of charges on coagulating particles which do not impede their agglomeration; the principal forces of solid particle agglomeration are electrostatic and molecular, with the final sizes at distances of r = 1 AU of 1 cm.

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